Ultraviolet (2000 A) galaxy counts: Comparison with predictions

Astronomy and Astrophysics – Astronomy

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

16

Astronomical Models, Galactic Evolution, Galactic Radiation, Spectral Energy Distribution, Spiral Galaxies, Star Formation, Stellar Spectrophotometry, Ultraviolet Astronomy, Color-Magnitude Diagram, Mathematical Models, Prediction Analysis Techniques, Stellar Color, Stellar Luminosity

Scientific paper

A prediction of galaxy counts at 2000 A and m2000 - B color distributions is elaborated from published spectral energy distributions and evolution models of galaxies. The comparison of the predictions to the observations at 2000 A is used to derive constraints on the local density of star-forming galaxies and their recent evolution. The data indicate a larger contribution of moderately blue ultraviolet-emitting galaxies than usually assumed in model counts at visible wavelengths. This discrepancy can reflect an underestimate of the local density of the actively star-forming galaxies, as well as an underestimate of the spectrophotometric and maybe numeric evolution of these objects. Models which call upon a large contribution of very blue galaxies to explain the well known number excess in galaxy counts near B = 18, produce blue tails in the m2000 - B color distributions which are not observed in the data.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Ultraviolet (2000 A) galaxy counts: Comparison with predictions does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Ultraviolet (2000 A) galaxy counts: Comparison with predictions, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Ultraviolet (2000 A) galaxy counts: Comparison with predictions will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1012643

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.